{"total":28,"items":[{"citing_arxiv_id":"2606.30307","ref_index":15,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The SKA-VLBI Perspective on Radio-Quiet AGN","primary_cat":"astro-ph.GA","submitted_at":"2026-06-29T13:49:06+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"Perspective outlining SKA-VLBI capabilities for resolving radio processes in radio-quiet AGN across kpc to sub-pc scales with sub-milliarcsecond imaging and μJy sensitivity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.27026","ref_index":10,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Unveiling the roles of thermal and nonthermal processes in the ISM & IGM structure formation and evolution of galaxies with SKAO","primary_cat":"astro-ph.GA","submitted_at":"2026-06-25T13:35:03+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26934","ref_index":19,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Unraveling the mysteries of supernovae with SKA+VLBI","primary_cat":"astro-ph.HE","submitted_at":"2026-06-25T12:08:43+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"SKA+VLBI will enable routine mas-scale imaging of nearby extragalactic supernovae to measure shock deceleration and test explosion mechanisms.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26914","ref_index":58,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Transforming X-ray Binary Astrophysics with SKA+VLBI","primary_cat":"astro-ph.HE","submitted_at":"2026-06-25T11:52:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"SKA+VLBI will deliver microarcsecond astrometry, polarimetry, and rapid multi-frequency imaging to track jets and accretion in X-ray binaries on AU scales.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.26223","ref_index":113,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Cross-correlation of SPT-3G D1 CMB lensing and DES Y3 galaxy lensing","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T18:00:01+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":7.0,"formal_verification":"none","one_line_summary":"Cross-correlation of SPT-3G D1 CMB lensing and DES Y3 galaxy lensing measures S8 = 0.833^{+0.047}_{-0.061} at 14 sigma using polarization-only reconstruction, consistent with Planck and DES Y3.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25955","ref_index":7,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Single-dish HI Intensity Mapping with the SKAO: Precursor Progress with MeerKAT's Large Area Synoptic Survey (MeerKLASS)","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T15:28:12+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"MeerKLASS reports successful single-dish HI intensity mapping detections that validate the technique for SKAO cosmology surveys.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25730","ref_index":26,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"The SKA View of Cool-core Clusters: Evolution of Radio Mini-halos and AGN Feedback","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T11:53:34+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"SKA-Mid all-sky surveys are projected to detect up to 3500 radio mini-halos at z<1 and enable a complete census of radio-loud BCGs to z~2.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25727","ref_index":27,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Probing High-redshift Intracluster Medium Using SKA","primary_cat":"astro-ph.CO","submitted_at":"2026-06-24T11:48:09+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Proposes SKA observations of El Gordo to study high-redshift ICM magnetic fields via continuum and polarization measurements and test amplification models.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25515","ref_index":31,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Accreting Compact Object Binaries with the SKA","primary_cat":"astro-ph.HE","submitted_at":"2026-06-24T07:48:14+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"This perspective paper outlines expected advances in studying accretion and jets in compact object binaries using the SKA's improved sensitivity and resolution.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25105","ref_index":28,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Bridging Theory and Observation in the SKA Era: A Cosmological Polarized Radiative Transfer Framework for Point-to-Point Polarized Sky Comparisons","primary_cat":"astro-ph.CO","submitted_at":"2026-06-23T19:22:31+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"A CPRT formalism is presented as a common platform to link cosmological MHD simulations, theory, and SKA polarized sky data for interpreting magnetic fields across cosmic time.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.25043","ref_index":3,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Evolution of AGN Across Cosmic Epochs with the SKAO","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T18:01:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"Simulated SKA-Mid surveys reach radio-AGN completeness at L_1.4GHz ~ 10^23 W Hz^-1 up to z~6.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.24810","ref_index":25,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect","primary_cat":"astro-ph.GA","submitted_at":"2026-06-23T16:57:27+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":3.0,"formal_verification":"none","one_line_summary":"SKA will enable Zeeman measurements of magnetic fields from cometary comas through Galactic structures and starburst galaxies to damped Ly-alpha systems at cosmological redshifts, with achievability tied to array assembly stages.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.17496","ref_index":7,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Effects of Rotation on the Gravitational Tug-Boat Mechanism for Neutron-Star Kicks and Implications for Spin-Kick Alignment","primary_cat":"astro-ph.HE","submitted_at":"2026-06-16T04:09:46+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A minimalist analytic extension shows spin-kick alignment in the tug-boat mechanism arises either from fast rotation averaging out perpendicular asymmetries or from spin-aligned mass flux, but the former requires unrealistically high rotation unless magnetic angular-momentum transport is efficient.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.05310","ref_index":48,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Decade to Map the Diffuse Universe: FRB-QSO Pairs with HST/COS Spectroscopy","primary_cat":"astro-ph.GA","submitted_at":"2026-06-03T18:02:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"Forecasts ~thousands of FRB-QSO pairs at <10' separation by 2035 for CGM, cosmic web, and Milky Way halo studies with HST/COS.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2606.02773","ref_index":70,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Why Little Red Dots Disappear at z < 3: Evolution of Number Density and Halo Mass","primary_cat":"astro-ph.GA","submitted_at":"2026-06-01T18:35:41+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"LRDs transition from underdense low-halo-mass environments at z>4 to typical galaxy conditions by z~3.5, with halo growth leading to larger sizes and SED changes that explain their disappearance at lower redshifts.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.22630","ref_index":79,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Towards precision cosmology with Void x CMB correlations (II): Impact of mock catalogs on the Void x CMB lensing signal","primary_cat":"astro-ph.CO","submitted_at":"2026-05-21T15:38:42+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Void x CMB lensing from Roman mocks is robust to catalog construction choices and forecasts S/N of 13-31 sigma with Planck, SO, and CMB-S4-like data for 2D and 3D voids.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.17460","ref_index":38,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"GRMHD Simulations of Magnetized Accretion Disk/Jet: Variabilities of Black Holes and Spectral Energy Distributions in Magnetic States","primary_cat":"astro-ph.HE","submitted_at":"2026-05-17T14:02:18+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"GRMHD simulations identify magnetic flux through the black hole horizon as the key variable setting jet efficiency and radiative output across MAD, INT, and SANE states, with mappings to temporal classes in GRS 1915+105 and other sources.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2605.06321","ref_index":198,"ref_count":2,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications","primary_cat":"astro-ph.HE","submitted_at":"2026-05-07T14:20:17+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":2.0,"formal_verification":"none","one_line_summary":"This review summarizes the theory, detection methods, and cosmological applications of gravitationally lensed gravitational waves from astrophysical sources such as compact binary mergers.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2604.18801","ref_index":38,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Preserving Clusters in Error-Bounded Lossy Compression of Particle Data","primary_cat":"cs.LG","submitted_at":"2026-04-20T20:10:54+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"A clustering-aware correction algorithm using spatial partitioning and projected gradient descent preserves single-linkage clusters in lossy-compressed particle data while keeping competitive compression ratios.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"In these contexts, the resulting clusters, including mass functions and spatial distributions, form the essential basis for high-level scientific inference. Thehalo mass function(HMF), denoted asdn/dlogM, represents the number density of dark matter halos per unit mass interval and serves as a critical downstream metric for validating cosmological simulations [38]. The HMF is a fundamental probe of theΛCold Dark Matter (ΛCDM) model, as its shape and evolution are directly governed by the growth of cosmic structures and the underlying dark matter density field [23], [39], [40]. For each identified haloi, we first calculate its total massM i; assuming uniform particle mass, Mi ∝N i, whereN i is the number of constituent particles"},{"citing_arxiv_id":"2604.11481","ref_index":47,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Emergence of Complex Web Structures","primary_cat":"astro-ph.CO","submitted_at":"2026-04-13T13:47:35+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":1,"top_context_role":"method","top_context_polarity":"use_method","context_text":"4 Top left: Two-dimensional slice through a three-dimensional cubic mesh containing a Gaus- sian random realization with a power spectrum that decays as a power law towards small scales. The box side length is 100h −1Mpc and the cell size is dL≃0.25h −1Mpc, withh= 0.677.Top right: Corresponding lognormal field constructed from the Gaussian realization shown in the top-left panel [47, 124].Bottom left: Field evolved dynamically with ridged augmented Lagrangian perturbation theory to redshiftz= 1.Bottom right: Potential associated with the evolved field in the bottom- left panel, obtained by applying the inverse Laplacian operator. The top-right panel shows that a local nonlinear mapping can alter the one-point distribution of the field, but does not reproduce"},{"citing_arxiv_id":"2604.11106","ref_index":57,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"On the origin of the BAOtr-DESI tension","primary_cat":"astro-ph.CO","submitted_at":"2026-04-13T07:23:08+00:00","verdict":"CONDITIONAL","verdict_confidence":"LOW","novelty_score":6.0,"formal_verification":"none","one_line_summary":"No CMB-consistent CPL dark energy model can simultaneously fit both the BAOtr and DESI datasets; the 3.7-sigma disagreement at z=0.51 sets an irreducible floor.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Karwal, M. Kamionkowski, Dark energy at early times, the Hubble parameter, and the string axiverse, Phys. Rev. D 94 (2016) 103523. arXiv:1608.01309,doi:10.1103/PhysRevD.94.103523. [56] A. G. Adame, et al., DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars, JCAP 04 (2025) 012.arXiv:2404.03000,doi: 10.1088/1475-7516/2025/04/012. [57] A. Carnero, E. Sánchez, M. Crocce, A. Cabré, E. Gaztañaga, Clus- tering of photometric luminous red galaxies - II. Cosmological impli- cations from the baryon acoustic scale, Mon. Not. Roy. Astron. Soc. 419 (2012) 1689-1694.arXiv:1104.5426,doi:10.1111/j.1365-2966. 2011.19832.x. [58] E. Sánchez, D. Alonso, F. J. Sánchez, J. García-Bellido, I. Sevilla,"},{"citing_arxiv_id":"2604.08175","ref_index":44,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"How many VHE gamma-ray binaries with young pulsars can be observed?","primary_cat":"astro-ph.HE","submitted_at":"2026-04-09T12:32:10+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":4.0,"formal_verification":"none","one_line_summary":"Population synthesis of pulsar-massive star binaries yields an estimate for the number of observable VHE gamma-ray sources in the Galaxy, incorporating anisotropic wind-interaction zones.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"Kuranov, S. B. Popov, K. A. Postnov, Pulsar spin-velocity alignment from single and binary neutron star progenitors, MNRAS 395 (2009) 2087-2094. doi: 10.1111/j.1365-2966. 2009.14595.x. arXiv:0901.1055. [43] V . M. Lipunov, K. A. Postnov, M. E. Prokhorov, The Scenario Machine: restrictions on key param- eters of binary evolution., A&A 310 (1996) 489- 507. [44] V . M. Lipunov, K. A. Postnov, M. E. Prokhorov, A. I. Bogomazov, Description of the \"Sce- nario Machine\", Astronomy Reports 53 (2009) 915-940. doi: 10.1134/S1063772909100047. arXiv:0704.1387. [45] C.-A. Faucher-Giguère, V . M. Kaspi, Birth and Evolution of Isolated Radio Pulsars, ApJ 643 (2006) 332-355. doi: 10.1086/501516. arXiv:astro-ph/0512585."},{"citing_arxiv_id":"2604.06792","ref_index":9,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Habitability Study of Terrestrial Planets: Application to Venus-like Worlds","primary_cat":"astro-ph.EP","submitted_at":"2026-04-08T07:57:50+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The authors introduce the Venus Similarity Index (VSI), Ancient Venus Similarity Index (AVSI) and Future Earth Similarity Index (FESI) as geometric-mean metrics to compare exoplanets to Venus-like environments for habitability studies.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2512.25040","ref_index":103,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Towards precision cosmology with Voids x CMB correlations (I): Roman-Agora mock catalogs and pipeline validation","primary_cat":"astro-ph.CO","submitted_at":"2025-12-31T18:37:53+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"The authors introduce analog matching to generate Roman Space Telescope mock catalogs that reproduce emission-line galaxy statistics and highlight the need to match void properties separately from two-point clustering for CMB cross-correlation studies.","context_count":1,"top_context_role":"background","top_context_polarity":"background","context_text":"algorithms into three categories: density-based, which identify underdense regions using smoothed density fields and often as- sume spherical shaped voids (Sánchez et al. 2017; Paz et al. 2023); geometrical-based finders, which use tessellation tech- niques to rely on the topology of the density field and do not make assumptions about void geometries (Platen et al. 2007; Neyrinck 2008); and dynamical-based, which rely on the dy- namics of the matter distribution through the displacement or velocity fields (Lavaux & Wandelt 2010). Studies are actively working to bridge the gap between the theoretical and the observational definition (Nadathur & Article number, page 8 of 19 Mar Pérez Sar et al.: Towards precision cosmology with Roman V oid×CMB correlations"},{"citing_arxiv_id":"2512.05584","ref_index":16,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Stellar feedback drives the baryon deficiency in low-mass galaxies","primary_cat":"astro-ph.GA","submitted_at":"2025-12-05T10:10:36+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Stacking DESI spectra reveals star-formation-driven Mg II outflows from low-mass galaxies that escape dark matter halos, providing indirect evidence that stellar feedback causes baryon deficiency.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2511.09311","ref_index":18,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales","primary_cat":"hep-ph","submitted_at":"2025-11-12T13:22:30+00:00","verdict":null,"verdict_confidence":null,"novelty_score":null,"formal_verification":null,"one_line_summary":null,"context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2510.24143","ref_index":46,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"Effects of tidal charge on Blandford-Znajek process around braneworld black holes","primary_cat":"gr-qc","submitted_at":"2025-10-28T07:35:45+00:00","verdict":"UNVERDICTED","verdict_confidence":"LOW","novelty_score":5.0,"formal_verification":"none","one_line_summary":"Positive tidal charge reduces Blandford-Znajek power by up to 15.2% while negative tidal charge increases it by up to 66.5% compared to Kerr black holes of equal mass and angular velocity.","context_count":0,"top_context_role":null,"top_context_polarity":null,"context_text":null},{"citing_arxiv_id":"2506.20707","ref_index":116,"ref_count":1,"confidence":0.88,"is_internal_anchor":false,"paper_title":"SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field","primary_cat":"astro-ph.CO","submitted_at":"2025-06-25T18:00:00+00:00","verdict":"ACCEPT","verdict_confidence":"MODERATE","novelty_score":6.0,"formal_verification":"none","one_line_summary":"SPT-3G delivers the most precise CMB EE and TE spectra at high multipoles to date, giving LCDM parameters with H0 = 66.66 ± 0.60 km/s/Mpc from ground-based data alone and reaching Planck-level constraints when combined with ACT.","context_count":1,"top_context_role":"dataset","top_context_polarity":"use_dataset","context_text":"23 AsPlanckdata are based on full sky observations, the fraction of these (small) correlations were shown to have a negligible effect on cosmological parameters in [40]. We further contextualize our results using non-CMB data. Here, we draw on the latest BAO measurements from DESI DR2 data [3]. We also consider the SDSS BAO data [111-114] and SNe Ia data from the Pantheon+ data set [116]. B. Constraints from CMB data In the following, we present constraints from CMB data alone. First, we verify the consistency of the SPT-3G D1 T&EdatawiththeΛCDMmodel(§VIIB1). We then report results for SPT alone and in combination with other CMB data (§VIIB2). Next, we explore exten- sions to theΛCDM model, beginning with an assessment of the internal consistency of CMB data with respect to"}],"limit":50,"offset":0}